{"id":4706,"date":"2015-09-08T00:00:00","date_gmt":"2015-09-07T15:00:00","guid":{"rendered":"http:\/\/www-v2.icrr.u-tokyo.ac.jp\/prwps\/news_en\/4706\/"},"modified":"2019-09-26T16:48:10","modified_gmt":"2019-09-26T07:48:10","slug":"new-data-direct-dark-matter-search-by-annual-modulation","status":"publish","type":"news_en","link":"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/news_en\/4706\/","title":{"rendered":"New Data: Direct Dark Matter Search by Annual Modulation"},"content":{"rendered":"<p> The XMASS experiment conducted a search for dark matter by means of the annual modulation caused by the earth&#8217;s rotation around the sun. The data used for this analysis was accumulated between November-2013 and March-2015.<\/p>\n<p> For more details, please see the pdf:<br \/>\n &gt; <a href=\"http:\/\/www-sk.icrr.u-tokyo.ac.jp\/xmass\/whatsnew\/whatsnew-20150907.pdf\">Direct Dark Matter Search by Annual Modulation<\/a><br \/>\n &gt; <a href=\"http:\/\/www-sk.icrr.u-tokyo.ac.jp\/xmass\/prelist\/20150907-kobayashi_darkmatterAc.pdf\">Presentation file at TAUP2015 conference<\/a><\/br><\/br><\/p>\n","protected":false},"featured_media":0,"template":"","taxo_news_en":[69,71],"class_list":["post-4706","news_en","type-news_en","status-publish","hentry","taxo_news_en-information","taxo_news_en-topics","en-US"],"aioseo_notices":[],"_links":{"self":[{"href":"https:\/\/www.icrr.u-tokyo.ac.jp\/wp-json\/wp\/v2\/news_en\/4706","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.icrr.u-tokyo.ac.jp\/wp-json\/wp\/v2\/news_en"}],"about":[{"href":"https:\/\/www.icrr.u-tokyo.ac.jp\/wp-json\/wp\/v2\/types\/news_en"}],"wp:attachment":[{"href":"https:\/\/www.icrr.u-tokyo.ac.jp\/wp-json\/wp\/v2\/media?parent=4706"}],"wp:term":[{"taxonomy":"taxo_news_en","embeddable":true,"href":"https:\/\/www.icrr.u-tokyo.ac.jp\/wp-json\/wp\/v2\/taxo_news_en?post=4706"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}